Evolutionary sequences of rotating protoneutron stars

Details Evolutionary sequences of rotating protoneutron stars Evolutionary sequences of rotating protoneutron stars

2003-10-30

arxiv.org/abs/astro-ph/0310875v2

Astron.Astrophys. 418 (2004) 283-294

Astronomy and Astrophysics

Astrophysics

14 pages, version accepted in A&A

Scientific paper

10.1051/0004-6361:20035619

We investigate the evolution of rigidly and differentially rotating protoneutron stars (PNSs) during the first twenty seconds of their life. We solve the equations describing stationary axisymmetric configurations in general relativity coupled to a finite temperature, relativistic equation of state, to obtain a sequence of quasi-equilibrium configurations describing the evolution of newly born neutron stars. Our estimates show that the scale of variation of the angular velocity in a PNSs is of the order of 7-10 km. We obtain the maximum rotation frequency that can be reached as the protoneutron stars deleptonizes and cools down, as well as other relevant parameters such as total angular momentum or |T/W|. Our study shows that imposing physical constraints (conservation of baryonic mass and angular momentum) and choosing reasonable thermodynamical profiles as the star evolves gives results consistent with the energetics of more complex simulations of non-rotating PNSs. It appears to be unlikely that PNSs formed in nearly axisymmetric core collapse reach the critical angular velocity to undergo the bar mode instability. They could, however, undergo secular or low |T/W| rotational instabilities a few seconds after birth, resulting in a strong emission of gravitational waves retarded with respect to the neutrino luminosity peak. We also found that the geometry of strongly differentially rotating protoneutron stars can become toroidal-like for large values of the angular velocity, before reaching the mass shedding limit.

Affiliated with

Also associated with

No associations

Rating

Evolutionary sequences of rotating protoneutron stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evolutionary sequences of rotating protoneutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolutionary sequences of rotating protoneutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-250188